{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:4F7YA5KH3IQXEMUJHVDTGVBGOR","short_pith_number":"pith:4F7YA5KH","schema_version":"1.0","canonical_sha256":"e17f807547da217232893d473354267479e037b253d46f4a993a771410b92a73","source":{"kind":"arxiv","id":"0709.4570","version":1},"attestation_state":"computed","paper":{"title":"Gamma-Ray Emission from PWNe Interacting with Molecular Clouds","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"H. Bartko, W. Bednarek","submitted_at":"2007-09-28T10:32:59Z","abstract_excerpt":"We consider a situation in which a pulsar (and its nebula) is formed inside or close to a high density regions of a molecular cloud. We apply a recent model for the gamma radiation of pulsar wind nebulae (PWN), which includes not only radiation processes due to injected leptons but also processes due to injection of relativistic hadrons, in order to calculate the expected gamma-ray emission from such interacting PWNe. The example calculations have been performed for two objects of this type from which directions TeV gamma-ray sources have recently been observed (IC443 and W41). We show that th"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"0709.4570","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-09-28T10:32:59Z","cross_cats_sorted":[],"title_canon_sha256":"80e79ec8e8df8dc619617742e68cdc6ad62e2fe24da7feca4ac32056f7acbf07","abstract_canon_sha256":"0e422e8d049a546dc11609f0d3db38b452ae729209837b1932b2c2ed4383fac9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:20:33.311160Z","signature_b64":"mFM0/cukPppMlwJuuaEkNUGBLdrG7+qHqB/MB20DyfopWrHE2Q2/AUxaZ2fw0Z02wsClYZ3zmqrnxRK3kqsfBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e17f807547da217232893d473354267479e037b253d46f4a993a771410b92a73","last_reissued_at":"2026-05-18T03:20:33.310225Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:20:33.310225Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma-Ray Emission from PWNe Interacting with Molecular Clouds","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"H. Bartko, W. Bednarek","submitted_at":"2007-09-28T10:32:59Z","abstract_excerpt":"We consider a situation in which a pulsar (and its nebula) is formed inside or close to a high density regions of a molecular cloud. We apply a recent model for the gamma radiation of pulsar wind nebulae (PWN), which includes not only radiation processes due to injected leptons but also processes due to injection of relativistic hadrons, in order to calculate the expected gamma-ray emission from such interacting PWNe. The example calculations have been performed for two objects of this type from which directions TeV gamma-ray sources have recently been observed (IC443 and W41). We show that th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0709.4570","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"0709.4570","created_at":"2026-05-18T03:20:33.310376+00:00"},{"alias_kind":"arxiv_version","alias_value":"0709.4570v1","created_at":"2026-05-18T03:20:33.310376+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0709.4570","created_at":"2026-05-18T03:20:33.310376+00:00"},{"alias_kind":"pith_short_12","alias_value":"4F7YA5KH3IQX","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_16","alias_value":"4F7YA5KH3IQXEMUJ","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_8","alias_value":"4F7YA5KH","created_at":"2026-05-18T12:25:54.717736+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR","json":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR.json","graph_json":"https://pith.science/api/pith-number/4F7YA5KH3IQXEMUJHVDTGVBGOR/graph.json","events_json":"https://pith.science/api/pith-number/4F7YA5KH3IQXEMUJHVDTGVBGOR/events.json","paper":"https://pith.science/paper/4F7YA5KH"},"agent_actions":{"view_html":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR","download_json":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR.json","view_paper":"https://pith.science/paper/4F7YA5KH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0709.4570&json=true","fetch_graph":"https://pith.science/api/pith-number/4F7YA5KH3IQXEMUJHVDTGVBGOR/graph.json","fetch_events":"https://pith.science/api/pith-number/4F7YA5KH3IQXEMUJHVDTGVBGOR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR/action/storage_attestation","attest_author":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR/action/author_attestation","sign_citation":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR/action/citation_signature","submit_replication":"https://pith.science/pith/4F7YA5KH3IQXEMUJHVDTGVBGOR/action/replication_record"}},"created_at":"2026-05-18T03:20:33.310376+00:00","updated_at":"2026-05-18T03:20:33.310376+00:00"}